Observation of B^{0}\to D^{*-}\tau^{+}\nu_{\tau} decay at Belle

  Observation of decay at Belle

Abstract

We report an observation of the decay in a data sample containing pairs collected with the Belle detector at the KEKB asymmetric-energy collider. We find a signal with a significance of 5.2 and measure the branching fraction . This is the first observation of an exclusive decay with a transition.

pacs:
13.20.He, 14.40.Nd

The Belle Collaboration

meson decays with transitions can provide important constraints on the Standard Model (SM) and its extensions. Due to the large mass of the lepton in the final state these decays are sensitive probes of models with extended Higgs sectors Itoh () and provide observables sensitive to new physics, such as polarizations, which cannot be accessed in other semileptonic decays.

Multiple neutrinos in the final states make the search for semi-tauonic decays very challenging and hence there is little experimental information about these processes. So far, results are limited to inclusive and semi-inclusive measurements by LEP experiments lep () which measure an average branching fraction of PDG (). SM calculations predict branching fractions for around 1.4% with uncertainties arising mainly from assumptions about form-factors hwang ().

In this paper we present the first observation of CC () decay using a data sample containing pairs that were collected with the Belle detector at the KEKB asymmetric-energy (3.5 on 8 GeV) collider KEKB () operating at the resonance ( GeV). The Belle detector is a large-solid-angle magnetic spectrometer consisting of a silicon vertex detector, a 50-layer central drift chamber, a system of aerogel Cherenkov counters, time-of-flight scintillation counters and an electromagnetic calorimeter (ECL) comprised of CsI(Tl) crystals located inside a superconducting solenoid coil that provides a 1.5 T magnetic field. An iron flux-return located outside the coil is instrumented to identify mesons and muons. A detailed description of the detector can be found in Ref. Belle (). We use Monte Carlo (MC) simulations to estimate signal efficiencies and background contributions. Large samples of the signal decays are generated with the EvtGen package evtgen () using the ISGW2 model isgw2 (). Radiative effects are modeled by the PHOTOS code photos (). MC samples equivalent to about twice the accumulated data are used to evaluate the background from and continuum () events.

decays to multi-neutrino final states can be observed at B-factories via the recoil of the accompanying meson () Ikado (). Reconstruction of the strongly suppresses the combinatorial and continuum backgrounds and provides kinematical constraints on the signal meson (). In this study we take advantage of the clean signature provided by the meson occurring on the signal side and reconstruct the “inclusively” from all the particles that remain after selecting candidates for daughters. We apply the analysis to decay chains that combine a high reconstruction efficiency with a low background level. The mesons are reconstructed in the decay channel. The ’s are reconstructed in the and final states. The and modes are used to reconstruct lepton candidates. We do not include the mode because in the relevant momentum range the muon identification is inefficient. The channel has higher combinatorial background than the purely leptonic mode, but the single neutrino in decay provides better kinematical constraints. For this mode we analyze only the decay.

We select charged tracks with impact parameters that are consistent with an origin at the beam spot, and having momenta above 50 MeV/ in the laboratory frame. Muons, electrons, charged pions, kaons and (anti)protons are identified using information from particle identification subsystems. The electrons from signal decays are selected with an efficiency greater than 90% and a misidentification rate below 0.2%. The momenta of particles identified as electrons are corrected for bremsstrahlung by adding photons within a 50 mrad cone along the trajectory. The candidates are reconstructed from photon pairs having invariant mass in the range 118 MeV/150 MeV/. From candidates that share a common , we select the with the smallest value from a mass-constrained fit. To reduce the combinatorial background, we require photons from the to have energies above 60 MeV -120 MeV, depending on the photon’s polar angle. Photons that do not come from a and exceed a polar-angle dependent energy threshold (100 MeV - 200 MeV) are included in the reconstruction.

We reconstruct the signal decay by selecting combinations of a meson and an electron or a pion candidate with opposite charge. We accept candidates with invariant masses in a 5 window around the nominal PDG PDG () value. candidates are accepted if the mass difference is in a 3 window around the PDG value. In order to reduce background from incorrectly reconstructed tracks, we impose tighter impact parameter requirements on the and candidates from decay.

Once a candidate is found, the remaining particles are used to reconstruct the decay. The consistency of a candidate with a -meson decay is checked using the beam-energy constrained mass and the energy difference variables: , and , where is the beam energy and and denote the momentum vector and energy of the ’th particle in the rest frame. The summation is over all particles that are not assigned to and satisfy the selection criteria described above. We require that events have at least one () pair and that and satisfy 5.2 GeV/ and 0.6 GeV. To improve the quality of the reconstruction, we impose the following requirements: zero total event charge, no and no additional in the event, zero net proton/antiproton number, residual energy in the ECL (i.e. the sum of energies of clusters that do not fulfill the requirements imposed on photons) less than 0.35 GeV and number of neutral particles on the tagging side 5. These criteria, which we refer to as “the -selection”, reject events in which some particles were undetected and suppress events with a large number of spurious showers. In order to validate the simulation and reconstruction, we use a control sample of events, where the decays to (followed by , ) which allows us to select a sample with a purity of 96% and with and daughters properly assigned to the parent particles. Figure 1 shows the and distributions of the control sample for data and the MC simulation scaled to the integrated luminosity in data. The events satisfy the -selection criteria and are in the GeV 0.05 GeV (for Fig. 1(a)) and 5.27 GeV/ (for Fig. 1(b)) windows. The good agreement of the shapes and of the absolute normalization demonstrates the validity of the MC-simulations for decays. Based on this study we constrain all further analysis to the region GeV0.05 GeV. With this requirement about 80% of the events are contained in the range GeV/.

Figure 1: and distributions for control sample from data (points with error bars) and MC (histograms).

The procedure described above, when applied to events with () pairs selects a relatively clean sample of semileptonic decays with the dominant non-signal contribution from the mode. Combinatorial background from hadronic -decays dominates in the mode. The background suppression exploits observables that characterize the signal decay: missing energy ; visible energy , i.e. the sum of the energies of all particles in the event; the square of missing mass and the effective mass of the () pair, where . The most powerful variable for separating signal and background is obtained by combining and () pair momentum: where is the mass. The variable is closely related to the missing mass in the decay and does not depend on reconstruction. It lies in the range for events with zero missing mass (e.g. with a single neutrino) and takes larger values if there are multiple neutrinos. The MC distributions of and for signal and background events after -selection for the mode are shown in Fig. 2. The relative normalizations of the main background categories, , , other decays and continuum, are determined from the data using looser selection criteria and verified using the sideband regions of the data sample that passed the final signal selection.

Figure 2: and distributions (normalized to unity) after the -selection for signal (blank) and background (shaded) for the mode in the region GeV/. The background components, from top to bottom: , , and other decays. The contribution from -continuum is negligible.

We optimize selection criteria using MC samples for signal and backgrounds, separately for decay chains with and with . In the first case we require 2.75, 1.9 GeV2.6 GeV and 8.3 GeV. We also reject events with a small difference between and to suppress background from hadronic decays where a genuine meson is combined with a soft secondary . Decays in the mode are selected by requiring 1.5, 0 ( and denote the masses of the and charged , respectively), 8.3 GeV, the energy of the from the () pair greater than 0.6 GeV, no in the event and less than four tracks that do not satisfy the requirements imposed on the impact parameters. The second requirement is equivalent to the condition 1, where denotes the angle between the two neutrinos in the () rest frame. The last three criteria reduce combinatorial background from low momentum pions and background from hadronic and decays. The above requirements result in flat distributions for most background components, while the signal distribution remains unchanged. This allows us to use the variable to extract the signal.

The distribution of the signal is described using a Crystal Ball (CB) lineshape function CB (). The shape parameters of the CB-function are determined from unbinned maximum likelihood fits to the combined MC signal samples. All the fits are performed in the range GeV/. The backgrounds are modeled as the sum of a combinatorial component using a parameterization introduced by ARGUS (ARGUS-function) ARGUS () and a peaking background described by the CB-function with shape parameters fixed from the fit to the signal MC. The main source of the peaking background is the semileptonic decay . Cross-feed events from signal decays followed by decays to other modes are negligible in the mode, but give significant contributions to the mode. About half of the cross-feed comes from decay. We parameterize the distribution of cross-feed events as a sum of CB and ARGUS functions with shape parameters fixed from fits to the signal and combinatorial background as described above. The component described by the CB-function is treated as a part of the signal. The efficiencies of signal reconstruction and the expected combinatorial and peaking backgrounds are given in Table 1.

The selection criteria established in the MC studies are applied to the data. The resulting distribution for data in all three decay chains is shown in Fig. 3. The overlaid histogram represents the expected background, scaled to the data luminosity. A clear excess over background can be observed.

Figure 3: distribution for the combined data sample. The histogram represents expected background scaled to the data luminosity. The solid curve shows the result of the fit. The dotted and dashed curves indicate respectively the fitted background and the component described by the ARGUS-function.

We extract signal yields by fitting the distributions to the sum of the expected signal and background distributions using the following likelihood function:

(1)

where is the in the ’th event and is the total number of events in the data. () denotes the signal (background) probability density function (PDF), which is parameterized as a CB (ARGUS)-function with shape parameters determined from fits to MC samples and , , and are the numbers of signal, combinatorial background and peaking background respectively. and are free parameters of the fit, while is fixed to the value obtained from fits to MC samples and scaled to the data luminosity ( is set to zero for the mode). The fits are performed both for the three decay chains separately and for all chains combined with a constraint to a common value of . The fit results are included in Table 1. The total number of signal events is with a statistical significance of 6.7. The significance is defined as , where and denote the maximum likelihood value and the likelihood value for the zero signal hypothesis. The fitted signal yield is used to calculate the branching fraction for the decay using the following formula, which assumes equal fractions of charged and neutral mesons produced in decays: , where is the number of pairs, denotes the reconstruction efficiency of the specific decay chain and is the product of intermediate branching fractions . All the intermediate branching fractions are set to the PDG values PDG (). The branching fraction obtained is %.

As a consistency check we also examine the distributions used in the signal selection, applying all requirements except those that are related to the considered variable. In all cases the distributions are well reproduced by the sum of signal and background components with normalizations fixed from the fits to the distribution. We also use the and (for mode) variables to extract the signal yield. We perform fits to distributions of these variables in the region GeV/ and obtain branching fractions in the range 1.83% - 2.05% and in agreement with the results from the fit.

subchannel B
, 40  4.59 5.0 0.79
,   60 17.03 2.6 0.50
, 148 25.72 3.8 0.48
Combined 248 47.34 6.7 0.57
Table 1: The number of expected combinatorial () and peaking () background events, number of signal () and combinatorial background () events determined by the fits, number of events in data (), signal selection efficiencies (), the product of the intermediate branching fractions (B), extracted branching fraction for (), statistical significance () and signal purity in the 5.27 GeV/ region. , and B in the mode include cross feed events. The listed errors are statistical only.

We consider the following sources of systematic uncertainties in the branching fraction determination. The systematic error on is 1.3%. The systematic uncertainties in the signal yield arise from uncertainties in the signal and background shape and peaking background. The systematic error due to the statistical uncertainties in the CB shape is 2.8%. The CB parameters obtained from MC-samples are, within statistical errors, consistent with those extracted from fits to the control sample in data. Therefore we do not introduce additional uncertainties due to imperfect signal shape modeling. The systematic errors due to the parameterization of the combinatorial background are evaluated by changing the ARGUS-shape parameters by . Fits with the shape parameters allowed to float provide consistent results within statistical uncertainties. The total systematic uncertainty due to the combinatorial background parameterization is %. The systematic error due to the peaking background is evaluated for each channel and amounts to % for combined modes, which is dominated by MC statistics. The effective efficiency includes uncertainties in determination of the efficiencies for reconstruction, () pair selection and signal selection. The uncertainty in reconstruction is taken as the statistical error in the efficiency evaluated from the data control sample (tagged with decay) and is 10.9%. The systematic error on the determination of () pair selection efficiency comes from systematic uncertainties in the tracking efficiency, neutral reconstruction efficiency and particle identification and is in the range 7.9%-10.7% depending on the decay chain. Systematic uncertainties in the signal selection efficiency are determined by comparing MC and data distributions in the variables used for signal selection. The uncertainties due to the partial branching ratios are taken from the errors quoted in the PDG PDG (). All of the above sources of systematic uncertainties are combined together taking into account correlations between different decay chains. The combined systematic uncertainty is 18.5%.

We include the effect of systematic uncertainty in the signal yield on the significance of the observed signal by convolving the likelihood function from the fit with a Gaussian systematic error distribution. The significance of the observed signal after including systematic uncertainties is 5.2.

In conclusion, in a sample of 535 pairs we observe a signal of 60 events for the decay with a significance of 5.2. This is the first observation of an exclusive decay with the transition. The measured branching fraction: % is consistent within experimental uncertainties with SM expectations hwang ().

We thank the KEKB group for excellent operation of the accelerator, the KEK cryogenics group for efficient solenoid operations, and the KEK computer group and the NII for valuable computing and Super-SINET network support. We acknowledge support from MEXT and JSPS (Japan); ARC and DEST (Australia); NSFC and KIP of CAS (China); DST (India); MOEHRD, KOSEF and KRF (Korea); KBN (Poland); MES and RFAAE (Russia); ARRS (Slovenia); SNSF (Switzerland); NSC and MOE (Taiwan); and DOE (USA).

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